When the eddy-driven jet is well seperated from the poleward edge of the Hadley cell the correlation approaches zero. These observations are seen in the aquaplanet model, the CMIP3 ensemble and reanalysis data, with a similar decrease in correlation over the same range of jet seperations suggesting a robust dynamical effect.
A dynamical mechanism is provided to explain the observed correlation patterns. It is well known in the literature that movement of the eddy-driven jet are sustained by anomalous upper tropospheric eddy-momentum flux convergence. These changes are approximately balanced by the Coriolis torque on the meridional flow, as expected under quasigeostrophic scaling. The location of the anomalous meridional mass flux, relative to the climatological Hadley cell position, determines the extent to which the edge of the Hadley cell is influenced by changes in the eddy-driven jet, and hence whether the two features are correlated.